Performance andPerformance and Operational Experience ...1.2E+19 r ated pot SPS extraction line:...

44
Performance and Performance and Operational Experience of Operational Experience of the CNGS Facility Edda GSCHWENDTNER, Dario AUTIERO, Karel CORNELIS, Ilias EFTHYMIOPOULOS, Alfredo FERRARI, Alberto GUGLIELMI, Ans PARDONS, Paola SALA Heinz VINCKE, Joerg WENNINGER (October 20, 2009)

Transcript of Performance andPerformance and Operational Experience ...1.2E+19 r ated pot SPS extraction line:...

  • Performance andPerformance and Operational Experience ofOperational Experience of

    the CNGS Facilityy

    Edda GSCHWENDTNER, Dario AUTIERO, Karel CORNELIS, Ilias EFTHYMIOPOULOS, Alfredo FERRARI, Alberto GUGLIELMI, Ans PARDONS, Paola SALA Heinz VINCKE, Joerg WENNINGER

    (October 20, 2009)

  • 22

    Outline

    • Introduction• Layout and Main Parameters• Operational Experience and PerformanceOperational Experience and Performance• Summary

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 3

    CERN Neutrinos to Gran Sasso (CNGS)Introduction

    ( )long base-line appearance experiment:

    • Produce muon neutrino beam at CERN• Measure tau neutrinos in Gran Sasso, Italy (732km) interaction in the target produces a lepton Identification of tau lepton by characteristic kink

    2 detectors in Gran Sasso:

    CERN • OPERA(1.2kton) emulsion target detector~146000 lead-emulsion bricks

    Gran Sasso • ICARUS(600ton) liquid argon TPC

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 4CNGS Facility – Layout and Main Parameters

    CNGS: Conventional Neutrino Beams

    + C K+

    Produce pions and Kaons to make neutrinos

    p + C (interactions) , K+ (decay in flight)

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 5

    targetmagnetichorns

    decay tunnel

    hadron absorber

    muon detector 1

    muon detector 2

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 6

    CERN Neutrinos to Gran SassoIntroduction

    CERN Neutrinos to Gran SassoApproved for 22.5 ·1019 protons on targeti 5 ith 4 5 1019 t/ 500mi.e. 5 years with 4.5·1019 pot/ year

    (200 days, nominal intensity)

    2.2·1017 pot/day

    500m

    2.2 10 pot/day ~1017 /day ~1011 /day at detector in Gran Sasso

    3600 i t ti / i OPERA 3600 interactions/year in OPERA(charged current interactions)

    2-3 interactions detected/year in OPERA Typical size of a detector at Gran Sassodetector at Gran Sasso1000m 3000m

    ~1 observed interaction with 2·1019 pot

    CNGS Run 2008: 1.78·1019 pot

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    Run 2009 today: 2.53·1019 pot

  • 7

    CNGS Proton Beam ParametersIntroduction

    Beam parameters Nominal CNGS beamNominal energy [GeV] 400

    Normalized emittance [m] H=12 V=7

    Emittance [m] H=0.028 V= 0.016

    Momentum spread p/p 0.07 % +/- 20%Momentum spread p/p 0.07 % / 20%

    # extractions per cycle 2 separated by 50 ms

    Batch length [s] 10.5500kW

    beam power# of bunches per pulse 2100

    Intensity per extraction [1013 p] 2.4

    Bunch length [ns] (4) 2g [ ] ( )

    Bunch spacing [ns] 5

    Beta at focus [m] hor.: 10 ; vert.: 20

    G 0 5Beam sizes at 400 GeV [mm] 0.5 mm

    Beam divergence [mrad] hor.: 0.05; vert.: 0.03

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    Expected beam performance: 4.5 x 1019 protons/year on target

  • 8

    CNGS ChallengesIntroduction

    g• High Intensity, High Energy Proton Beam

    (500kW, 400GeV/c)( , )– Induced radioactivity

    • In components, shielding, fluids, etc…– Intervention on equipment ‘impossible’

    • Remote handling by overhead crane• Replace broken equipment, no repair• Human intervention only after long ‘cooling time’

    – Design of equipment: compromise– Design of equipment: compromise• E.g. horn inner conductor: for neutrino yield: thin tube, for reliability: thick tube

    • Intense Short Beam Pulses, Small Beam Spot(up to 3.5x1013 per 10.5 s extraction, < 1 mm spot)– Thermo mechanical shocks by energy deposition (designing target rods,

    thin windows, etc…)

    Proton beam: Tuning, Interlocks!

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    most challenging zone: Target Chamber (target–horn–reflector)

  • 9

    CNGS Layout and Main Parameters

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 10

    CNGS Primary Beam LineCNGS Facility – Layout and Main Parameters

    CNGS Primary Beam Line100m extraction together with LHC, 620m long arc to bend towards Gran Sasso, 120m long focusing section

    Magnet System:• 73 MBG Dipoles

    – 1.7 T nominal field at 400 GeV/c• 20 Quadrupole Magnets

    – Nominal gradient 40 T/m• 12 Corrector Magnets

    Beam Instrumentation:• 23 Beam Position Monitors (Button Electrode BPMs)

    – recuperated from LEP– recuperated from LEP– Last one is strip-line coupler pick-up operated in air– mechanically coupled to target

    • 8 Beam profile monitorsp– Optical transition radiation monitors: 75 m carbon or 12 m titanium screens

    • 2 Beam current transformers• 18 Beam Loss monitors

    SPS t N fill d i i ti h b

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    – SPS type N2 filled ionization chambers

  • 11

    Primary Beam Line

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 12

    CNGS Secondary Beam LineCNGS Facility – Layout and Main Parameters

    43 4m2.7m

    TBID

    43.4m100m

    1095m 18m 5m 5m67mAir cooled graphite target

    – Target table movable horizontally/vertically for alignment

    • Multiplicity detector: TBID, ionization chambers

    • 2 horns (horn and reflector)2 horns (horn and reflector)– Water cooled, pulsed with 10ms half-sine wave pulse of up to 150/180kA, remote polarity change

    possible

    • Decay pipe: – 1000m, diameter 2.45m, 1mbar vacuum, 3mm Ti entrance window, 50mm carbon steel water cooled

    exit window.

    • Hadron absorber: – Absorbs 100kW of protons and other hadrons

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    Absorbs 100kW of protons and other hadrons

    • 2 muon monitor stations: muon fluxes and profiles

  • 13

    CNGS TargetTarget magazine: 1 unit used, 4 in-situ spares CNGS Facility – Layout

    13 graphite rods, each 10cm long,

    Ø = 5mm and/or 4mm

    2.7mm interaction length

    Ten targets (+1 prototype) have beenTen targets (+1 prototype) have been built. Assembled in two magazines.

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 14

    CNGS Horn and ReflectorCNGS Facility – Layout and Main Parameters

    0.35 m

    i d t

    • 150kA/180kA, pulsed• 7m long, inner conductor 1.8mm thick

    7

    inner conductor

    • Designed for 2·107 pulses• Water cooling to evacuate 26kW• 1 spare horn (no reflector yet)

    Design features• Water cooling circuit

    – In situ spare, easy switch•

  • 15

    Decay TubeDecay Tube

    – steel pipe– 1mbar

    994m long– 994m long– 2.45m diameter, t=18mm,

    surrounded by 50cm concrete – entrance window: 3mm Ti

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    – exit window: 50mm carbon steel, water cooled

  • 16CNGS Facility – Layout and Main Parameters

    M M it270cm• 2 x 41 fixed monitors

    Muon Monitors

    60cm270cm(Ionization Chambers)

    • 2 x 1 movable monitor

    11.25cm

    LHC type Beam Loss Monitorsyp• Stainless steel cylinder • Al electrodes, 0.5cm separation• N2 gas filling2 g g

    FermiLab, 20 October 2009Edda Gschwendtner, CERN CNGS

    • Muon Intensity:– Up to 8 107 /cm2/10.5s

  • 17

    Operational Experience andOperational Experience and Performance

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 18

    CNGS Timeline2000-2005 Civil Engineering & Installation CERN

    2006Beam Commissioning CERN

    2006:10 July-27 Oct

    g0.08· 1019 potDetector electronics

    commissioning Gran Sasso

    2006 2007 f2006-2007:Shutdown

    Reflector Water Leak Repair/Improvement CERN

    Beam Commissioning at high CERN2007:

    17 Sept-20 Octintensity

    0.08· 1019potDetector commissioning with 60000 bricks Gran Sasso

    2007-2008:Shutdown

    Additional shielding and electronics re-arrangement CERN

    Finishing OPERA bricks Gran SassoFinishing OPERA bricks Gran Sasso

    2008:18 June- 3 Nov

    CNGS Physics Run 1.78· 1019pot

    2009

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    2009:1 June-today

    CNGS Physics Run 2.4· 1019pot

  • 19

    CNGS PerformanceCNGS Performance

    CNGS Performance2008: 18 June – 3 November 2008• Excellent performance of the CNGS FacilityExcellent performance of the CNGS Facility• CNGS modifications finished successfully• Beam line equipment working well and stable

    1.78·1019 protons on target

    OPERA experiment:10100 ti t• 10100 on-time events

    • 1700 candidate interaction in bricks

    2009: 28 May – 23 November 2009 16nd October 2009: 2.53·1019 protons on target

    OPERA experiment:• >15500 on-time events• >2500 candidate interaction in bricks

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 20

    Supercycle 2008LHC

    CNGS Performance

    4x CNGS2xCNGS MTE/CNGS

    LHC

    50.4s supercycle: 7 CNGS, 1 LHC 83% CNGS duty cycle

    SFTPRO 3xCNGS LHC MD

    48s supercycle:North Area 3 CNGS 1LHC 1MD 83% CNGS duty cycleNorth Area, 3 CNGS, 1LHC,1MD 37.5% CNGS duty cycle

    Supercycle 200946.8s supercycle:

    4xCNGS

    46.8s supercycle:North Area, 4 CNGS, 1LHC 51.3% CNGS duty cycle

    LHC

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    SFTPROLHC

  • 21

    CNGS Run 2008: 18 June- 03 Nov 20081 8E 19

    CNGS Performance

    1.6E+19

    1.8E+19

    Total: 1 78·1019 pot

    CNGS maintenance

    1 2E+19

    1.4E+19Total: 1.78·1019 pot

    Nominal: 4.5 1019 pot/yr for 5 years

    1E+19

    1.2E+19

    rate

    d po

    t SPS extraction line: Magnet ground fault MD

    6E+18

    8E+18

    inte

    gr

    18kV cable

    SPS timing fault:vacuum leak & magnet exchange

    CNGS maintenance

    4E+18

    repairPS magnet exchange, septum bakeout MD

    0

    2E+18

    MD

    bakeout MD

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    18-J

    un

    28-J

    un

    8-Ju

    l

    18-J

    ul

    28-J

    ul

    7-A

    ug

    17-A

    ug

    27-A

    ug

    6-Se

    p

    16-S

    ep

    26-S

    ep

    6-O

    ct

    16-O

    ct

    26-O

    ct

    5-N

    ov

  • 22

    2009 Protons on TargetCNGS Performance

    2009 protons on target3.6E+19

    2009 Protons on TargetTotal POT expected 2009: 3.22E19

    2.8E+193E+19

    3.2E+193.4E+19

    rget

    Expected protons on targetAchieved protons on target

    Current expected pot: 2.47E19Current achieved pot: 2.53 E19

    T t l POT 2008 1 78E19

    PS septum

    2E+192.2E+192.4E+192.6E+19

    ons

    on ta

    r Total POT 2008: 1.78E19

    CNGS i t

    Linac vacuum leak

    repair

    1.2E+191.4E+191.6E+191.8E+19

    rate

    d pr

    oto

    UA9, SPS magnet exchange

    CNGSmaintenance

    maintenance MD

    4E+186E+188E+181E+19

    inte

    gr exchange, kicker repair

    MD

    MD

    02E+18

    2-M

    ay9-

    May

    5-Ju

    n2-

    Jun

    9-Ju

    n

    6-Ju

    n3-

    Jul

    0-Ju

    l

    7-Ju

    l24

    -Jul

    31-J

    ul

    7-A

    ug4-

    Aug

    1-A

    ug

    8-A

    ug4-

    Sep

    1-Se

    p

    8-Se

    p5-

    Sep

    2-O

    ct

    9-O

    ct6-

    Oct

    3-O

    ct

    0-O

    ct6-

    Nov

    3-N

    ov

    0-N

    ov7-

    Nov

    MD

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    22 29 5 12 19 26 1 1 2 3 7 14 21 28 4 11 18 252 9 16 23 30 6 13 20 27

  • 23

    SPS Efficiencies for CNGSCNGS Performance

    SPS Efficiencies for CNGS2008 2009

    Integrated efficiency: 60.94% Integrated efficiency: 69%

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 24

    Total Protons on Targetg

    4.0E+19

    4.5E+19

    2009

    3 0E 19

    3.5E+19

    2.5E+19

    3.0E+19

    rated po

    t

    2008

    1.5E+19

    2.0E+19

    integr

    a

    5 0E+18

    1.0E+19

    2006 2007

    0.0E+00

    5.0E+18

    y-06

    ul-06

    g-06

    ct-06

    c-06

    b-07

    pr-07

    n-07

    g-07

    ct-07

    c-07

    b-08

    pr-08

    n-08

    g-08

    ct-08

    c-08

    b-09

    pr-09

    n-09

    g-09

    ct-09

    c-09

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    May Jul

    Aug Oct

    Dec Feb

    Apr

    Jun

    Aug Oct

    Dec Feb

    Apr

    Jun

    Aug Oct

    Dec Feb

    Apr

    Jun

    Aug Oct

    Dec

  • 25

    Primary BeamCNGS Performance

    • Extraction interlock in LSS4 modified to accommodate the simultaneous operation of LHC and CNGS

    – Good performance, no incidents• No extraction and transfer line losses• Trajectory tolerance: 4mm, last monitors to +/-2mm and +/- 0.5mm (last 2 monitors)

    – Largest excursion just exceed 2mm• Total trajectory drift over 2008 is ~1mm rms in each plane

    Horizontal plane

    2mm

    Horizontal plane

    Vertical plane

    2mm

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 26

    Target Beam PositionCNGS Performance

    g• Excellent position stability; ~50 (100) m horiz(vert) over entire run.• No active position feedback is necessaryp y

    – 1-2 small steerings/week only

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    Horizontal and vertical beam position on the last BPM in front of the target

  • 27

    On-line Muon Profiles

    Horizontal, pit1 Horizontal, pit2

    Centroid for each profile and extraction

    V ti l it1

    • bl

    Vertical, pit2Vertical, pit1

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 28

    Beam Stability seen on Muon MonitorsCNGS Performance

    Beam Stability seen on Muon Monitors• Position stability of muon beam in pit 2 is ~2cm rms• Beam position correlated to beam position on targetBeam position correlated to beam position on target.

    – Parallel displacement of primary beam on T40

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 29

    Muon MonitorsCNGS Performance

    Very sensitive to any beam changes !– Offset of beam vs target at 0.05mm level Muon Profiles Pit 2

    1

    2

    3

    Centroid of horizontal profile pit2

    -2

    -1

    0

    cm

    5cm shift of muon profile centroid ~80m parallel beam shift

    -5

    -4

    -3

    c

    -8

    -7

    -6

    9 0:

    00

    9 0:

    28

    9 0:

    57

    9 1:

    26

    9 1:

    55

    9 2:

    24

    9 2:

    52

    9 3:

    21

    9 3:

    50

    9 4:

    19

    9 4:

    48

    9 5:

    16

    9 5:

    45

    9 6:

    14

    9 6:

    43

    Muon Profiles Pit 1

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    10/29

    – Offset of target vs horn at 0.1mm level• Target table motorized

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    Muon Profiles Pit 1• Horn and reflector tables not

  • 30

    Beam IntensityCNGS Performance

    y

    Typical transmission of the CNGS beam through the SPS cycle ~ 92%.Injection losses 6%

    Error : rms spread

    Injection losses ~ 6%.

    x 1010

    Protons on target/extraction

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 31

    Muon Detector Non-Linearity PuzzleCNGS Performance

    y2007: observation: non-linear muon detector signal in horizontal profile of pit 1

    (not in vertical profile, neither in profiles of pit 2)

    Looks like saturation effect

    ctor

    sig

    nal

    saturation effect But:

    Check:m

    uon

    dete

    c

    Timing?Electronics cards?Beam intensity?

    orm

    aliz

    ed m

    ch/p

    ot/e

    xtr) Beam intensity?

    N (c

    pot/extraction

    FermiLab, 20 October 2009Edda Gschwendtner, CERNA. Marsili et al, AB-2008-044-BI

  • 32

    Muon Detector Non-Linearity PuzzleCNGS Performance

    2008Wire topology:All detectors are connected to readout cardvia a 750m long twisted multi-wire cable.

    2009

    pot/e

    xtr)

    Horizontal profile detectors are inside themulti-wire cable

    See different capacitances!

    sign

    al (c

    h/p

    on d

    etec

    tor

    mal

    ized

    muo

    Remedy:

    Nor

    m

    pot/extraction

    yIncrease capacitance of all wires to a fixed value: adding 220nF capacitor between each

    ire and shielding

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    wire and shielding.

  • 33

    CNGS Polarity PuzzleCNGS Performance

    yMuon Detector Sensitive to any beam change (e.g. offset of beam vs target at 50m level)

    Online feedback on quality of neutrino beam

    • Observation of asymmetry in horizontal direction between

    N t i (f i f ith iti h )270cm

    q y

    – Neutrino (focusing of mesons with positive charge)– Anti-neutrino (focusing of mesons with negative

    charge)11.25cm

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 34

    CNGS Polarity PuzzleCNGS Performance

    Explanation: Earth magnetic field in 1km long decay tube!– calculate B components in CNGS reference system– Partially shielding of magnetic field due to decay tube steely g g y Results in shifts of the observed magnitude Measurements and simulations agree very well (absolute

    comparison within 5% in first muon pit)p p )

    NeutrinoFocusing on

    positive

    Anti-neutrinoFocusing on

    negative chargepositive charge

    negative charge

    a et

    al 2

    008

    Lines: simulated flux

    ulat

    ions

    , P. S

    al

    Points: measurementsNormalized to max=1

    FLU

    KA

    sim

    uFermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 35

    Muon Monitors: Measurements vs. SimulationsCNGS Performance

    pit 1 Horizontal

    0 3

    0.35

    0.4

    measurementsimulation

    Horizontal Profile Pit 1pit 2 Horizontal

    0.012

    0.014

    pot

    measurementsimulation

    Horizontal Profile Pit 2

    0.15

    0.2

    0.25

    0.3

    ch/p

    ot

    0.006

    0.008

    0.01 ch/p

    08

    0

    0.05

    0.1

    -157.5 -135 -112.5 -90 -67.5 -45 -22.5 0 22.5 45 67.5 90 112.5 135 157.5 0

    0.002

    0.004

    -157.5 -135 -112.5 -90 -67.5 -45 -22.5 0 22.5 45 67.5 90 112.5 135 157.5cmMeasurements ula

    tions

    200

    cm

    pit 1 Vertical

    0.35

    0.4

    measurementsimulation

    Vertical Profile Pit 1 pit 2 Vertical

    0.012

    0.014

    t

    measurementsimulation

    Vertical Profile Pit 2

    cmMeasurementsSimulations

    FLU

    KA

    sim

    0.2

    0.25

    0.3

    ch/p

    ot

    simulation

    0.006

    0.008

    0.01 ch/p

    o

    Sala

    et a

    l, F

    0

    0.05

    0.1

    0.15

    0

    0.002

    0.004

    P. S

    FermiLab, 20 October 2009Edda Gschwendtner, CERN Excellent agreement!

    0-157.5 -135 -112.5 -90 -67.5 -45 -22.5 0 22.5 45 67.5 90 112.5 135 157.5

    cm

    0-157.5 -135 -112.5 -90 -67.5 -45 -22.5 0 22.5 45 67.5 90 112.5 135 157.5

    cm

  • 36

    SummarySummary• CNGS commissioned in 2006• Successful modifications in the CNGS facility and completion

    of the OPERA Detector Ph i i 2008• Physics run since 2008– 2008:

    1 78 1019 t t t t t l• 1.78 1019 protons on target total

    – 2009: • Expect 3 2 1019 protons on target total• Expect 3.2 1019 protons on target total• Today (16 October 2009): 2.53 1019 protons on target

    Waiting for tau neutrino results!!

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 37

    • Additional Slides

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 38

    CNGS Performance - ReminderCNGS Facility – Performance Results 2008

    C GS e o a ce e de

    Examples: effect on ντ cc events

    horn off axis by 6mm < 3%horn off axis by 6mm < 3%reflector off axis by 30mm < 3%proton beam on target < 3%off axis by 1mmoff axis by 1mmCNGS facility misaligned < 3%by 0.5mrad (beam 360m off)

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 39

    Helium Tube Entrance Window0 3 thi k

    CNGS Facility – Experience of Operating a 500kW Facility

    Temperature Measurements

    – 0.3mm thick– 0.8m inner

    diameter– Clamped with seal

    shielding

    ionization chamber

    BPM w Clamped with seal between flanges

    shielding

    horntargetTBIDcollimator

    BPM

    beamHelium tube

    Ti-w

    indo

    w

    Temperature Measurement

    ionization chamber Clampingbolt

    SealTitanium Grade (Ti-6Al-4V)– Ultimate stress:

    – @20°C: >900MPa

    Entrance window

    @– @100°C: >870MPa– @150°C: >850MPa

    From calculations:- When ventilation vs. beam is such that temp. at flange = 66°C:Window: Temp

  • 40

    Helium Tube Entrance Window TemperatureCNGS Facility – Experience of Operating a 500kW Facility

    CNGS duty cycle: 37.5%, 54% 37.5%, 43% 37.5%,45%,54%

    56%-83%

    p

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

  • 41

    CNGS Radiation IssuesOperational Experience

    CNGS: no surface building above CNGS target area many electronics in tunnel area

    • During CNGS run 2007:During CNGS run 2007: – Failure in ventilation system installed in the CNGS tunnel area due to radiation effects in

    electronics (SEU due to high energy hadron fluence).• modifications during shutdown 2007/08:

    M f h l i f CNGS l– Move most of the electronics out of CNGS tunnel area– Create radiation safe area for electronics which needs to stay in CNGS– Add shielding 53m3 concrete up to 6m3 thick shielding walls

    106 h/cm2/yr2008++2006/07

    109 h/cm2/yr10 h/cm /yr

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    p-beam target chamber p-beam target chamber

  • 42

    Neutrino Parameter Status: July 2008 Review of Particle Physics

    Introduction

    If flavor eigenstates and mass eigenstates are different (mixing) and if masses are different neutrino oscillation

    Mass states: Flavor states:

    Mixing of the three neutrinos: unitary 3x3 matrix 4 parameters like the CKM matrix for Quarks. CP violating phase not yet accessible currently 3 mixing angles .

    ~

    m221 = 8 ± 0.3 x 10-5 eV2 m21 = 9 ± 0.17 meV solar and reactor Neutrinosm232 = 2.5 ± 0.5 x 10-3 eV2 m32 = 50 ± 5 meV Atmospheric and long Baseline

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    sin2223 > 0.93 23=35.3 degrees compatible with max. mixing =45 degrees

  • 43

    NeutrinosIntroduction

    Weakly interacting leptons e, no charge

    • Solar Neutrinos:– 6·1014 neutrinos/s/m2

    Every 100 years 1 neutrino interacts in human body 1016 meter lead to stop half of these neutrinos

    • Natural radioactivity from earth:Natural radioactivity from earth:– 6·106 neutrinos/s/cm2.

    • 40K in our body:– 3.4·108 neutrinos/day

    • Cosmic neutrinos:330 neutrinos/cm3– 330 neutrinos/cm3

    • CNGS

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    – Send ~1017 neutrinos/day to Gran Sasso

  • 44

    Neutrino IntroductionIntroduction

    m232… governs the to oscillation

    Up to now: only measured by disappearance of muon neutrinos:P d t i b t i fl t d t t• Produce muon neutrino beam, measure muon neutrino flux at near detector

    • Extrapolate muon neutrino flux to a far detector• Measure muon neutrino flux at far detector• Difference is interpreted as oscillation from muon neutrinos to undetected tau neutrinos K2K, NuMI

    CNGS (CERN Neutrinos to Gran Sasso): long base-line appearance experiment:g pp p

    • Produce muon neutrino beam at CERN• Measure tau neutrinos in Gran Sasso, Italy

    (732km) Very convincing verification of the neutrino CERN Very convincing verification of the neutrino

    oscillationCERN

    Gran Sasso interaction in the target produces a lepton interaction in the target produces a lepton Identification of tau lepton by characteristic kink2 detectors in Gran Sasso:• OPERA (1.2kton) emulsion target detector

    146000 l d l i b i k

    FermiLab, 20 October 2009Edda Gschwendtner, CERN

    ~146000 lead-emulsion bricks• ICARUS (600ton) liquid argon TPC